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Radio and X-ray observations of G11.2 - 0.3 and G41.1 - 0.3The supernova remnants G11.2 - 0.3 and G41.1 - 0.3 have been observed in radio and X-ray utilizing the VLA and Einstein Observatory, respectively. The acquired images reveal that both sources have shell morphologies and do not exhibit any clear indication of a central stellar remnant. In addition, both objects are relatively bright X-ray sources.
Document ID
19860026127
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/163465
Authors
Becker, R. H. (California, University Davis, United States)
Markert, T. (California Univ. Davis, CA, United States)
Donahue, M. (MIT Cambridge, MA, United States)
Date Acquired
August 12, 2013
Publication Date
September 15, 1985
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 296
ISSN: 0004-637X
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-637X
Accession Number
86A10865
Funding Number(s)
CONTRACT_GRANT: NAG8-494
CONTRACT_GRANT: NSF AST-83-13685
CONTRACT_GRANT: NAG8-501
Distribution Limits
Public
Copyright
Other

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